HOW DO STARS DIE ? MAYUMI BARCENA AND JASMIN DE LEON.

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Presentation transcript:

HOW DO STARS DIE ? MAYUMI BARCENA AND JASMIN DE LEON

STARS massive SUN

end of productive phase Chandrasekhar Limit WHITE DWARF

CHANDRASEKAHAR LIMIT stable white dwarf 1.4 Subrahmanyan Chandrasekhar Wilhelm Anderson and E.C. Stoner the limit,ignored logically require black hole

NEUTRON STAR created,4-8 solar masses undergo supernova explosion remaining protons and electrons

SUPERNOVA stellar explosion radiating energy Sun expected to emit before fading hydrogen fusing

SUPERNOVA

BLACK HOLE condense to black hole region of spacetime prevents anything stellar masses continue to grow supermassive black holes

BLACK HOLE

REFERENCES en.wikipedia.org/wiki/Chandrasekhar_limit en.wikipedia.org/wiki/Black_hole en.wikipedia.org/wiki/Subrahmanyan_Chandrasekhar www.superbwallpapers.com/fantasy/black_hole_26843 www.esa.int/Our_Activities/Space_Science/Stars_Neutron_Stars_pulsars_and_magnetars imagine.gsfc.nasa.gov/docs/ask_atro/answers/010607a.html www.universetoday.com/24186/how_does_a_star_die/ chandra.harvard.edu/resources/illustrations/stellar_evolution._html sky_is_full_of_shinning_stars_the_moon_walking_soft_and_gentle_light_wish_one_good_sleep_hd_natural_scenery_walpaper/ en.wikipedia.org/wiki/star en.wikipedia.org/wiki/Sun en.wikipedia.org/wiki/Neutron_star venturegalleries.com/blog/finding_my_writing_place_in_the_universe/

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